Fig. 4.
As in the left panel of Fig. 3, but for the central dust-to-gas mass ratios vs. central cold gas masses, where the H I measurements are from the central regions of the galaxies only (≈35″ × 45″; Young et al. 2014). Data points are colour-coded according to the galaxies’ specific stellar angular momenta (fast- and slow-rotators; left) and CO morphologies (Alatalo et al. 2013; right).
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